Greta Stacy is a high school science teacher in Doha, Qatar. She has previously taught in Ecuador and the United States.
Teaching about fusion energy provides a great way to connect the study of atomic theory to climate change and make learning relevant for students. Beginning with an explanation of fusion power can be helpful. This can allow students to consider fusion energy in comparison with other forms of green energy and climate change solutions. This lesson for high school students allows students to take a deeper dive and conduct their own research on fusion energy.
Written By: MIT Environmental Solutions Initiative
The MIT Climate Change Engagement Program, a part of MIT Climate HQ, provides the public with nonpartisan, easy-to-understand, and scientifically-grounded information on climate change and its solutions.
Fusion energy is the source of energy at the center of stars, including our own sun. Stars, like most of the universe, are made up of hydrogen, the simplest and most abundant element in the universe, created during the big bang. The center of a star is so hot and so dense that the immense pressure forces hydrogen atoms together. These atoms are forced together so strongly that they create new atoms entirely—helium atoms—and release a staggering amount of energy in the process. This energy is called fusion energy.
More energy than chemical energy
Fusion energy, like fossil fuels, is a form of stored energy. But fusion can create 20 to 100 million times more energy than the chemical reaction of a fossil fuel. Most of the mass of an atom, 99.9 percent, is contained at an atom’s center—inside of its nucleus. The ratio of this matter to the empty space in an atom is almost exactly the same ratio of how much energy you release when you manipulate the nucleus. In contrast, a chemical reaction, such as burning coal, rearranges the atoms through heat, but doesn’t alter the atoms themselves, so we don’t get as much energy.
